粗语
发表于 2025-3-28 15:39:49
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愤慨点吧
发表于 2025-3-28 18:49:55
https://doi.org/10.1007/978-3-031-17933-4al region is associated with a dense molecular gas disk, in which the majority of gas is concentrated in a rotating molecular ring. Outflow structures like the radio lobe is associated with rotating molecular gas at high speed, consistent with a twisted magnetic cylinder driven by accretion of a rotating gas disk.
comely
发表于 2025-3-28 23:17:31
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唠叨
发表于 2025-3-29 03:20:31
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不要严酷
发表于 2025-3-29 09:56:41
The barred galaxy NGC 1530, identify with large scale shocks observed in hydrodynamic simulations. Although hydrodynamical models are generally used to constrain the mass model, the observations could in turn be used to find a better ISM descriptor.
猛然一拉
发表于 2025-3-29 13:17:11
A circumnuclear molecular torus in NGC 1365, 5″ is the dominant feature. Molecular emission is also seen coming from various dust streamers in the bar of the galaxy. The velocity field of the molecular region agrees well with predictions of models of gas streaming in the bar and nuclear region.
询问
发表于 2025-3-29 17:50:16
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舰旗
发表于 2025-3-29 20:19:22
Radio continuum and molecular gas in the Galactic Center,al region is associated with a dense molecular gas disk, in which the majority of gas is concentrated in a rotating molecular ring. Outflow structures like the radio lobe is associated with rotating molecular gas at high speed, consistent with a twisted magnetic cylinder driven by accretion of a rotating gas disk.
Arroyo
发表于 2025-3-30 00:34:47
Conference proceedings 1996etical papers describe their evolution, the dynamics as well as fundamental physical effects near their nuclei. Other contributions cover numerical and observational aspects and thus represent a very active area in astrophysics. The centre of our galaxy was also amply dealt with. The collection addresses researchers as well as graduate students.
FICE
发表于 2025-3-30 06:55:19
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